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  2. Kappa Centauri - Wikipedia

    en.wikipedia.org/wiki/Kappa_Centauri

    As of 2007, the secondary component was separated from the primary by 0.128 arcseconds at a position angle of 156°. It has about 68% of the mass of the primary. [ 9 ] This system is a proper motion member of the Upper Centaurus–Lupus sub-group in the Scorpius–Centaurus OB association , the nearest such co-moving association of massive ...

  3. List of nearest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars

    This number is likely much higher, due to the sheer number of stars needed to be surveyed; a star approaching the Solar System 10 million years ago, moving at a typical Sun-relative 20–200 kilometers per second, would be 600–6,000 light-years from the Sun at present day, with millions of stars closer to the Sun.

  4. HD 141569 - Wikipedia

    en.wikipedia.org/wiki/HD_141569

    HD 141569 is an isolated [5] Herbig Ae/Be star [6] of spectral class A2Ve [7] approximately 364 light-years away in the constellation of Libra. The primary star has two red dwarf companions (orbiting each other) at about nine arcseconds. In 1999, a protoplanetary disk was discovered around the star.

  5. Light-year - Wikipedia

    en.wikipedia.org/wiki/Light-year

    The product of Simon Newcomb's J1900.0 mean tropical year of 31 556 925.9747 ephemeris seconds and a speed of light of 299 792.5 km/s produced a light-year of 9.460 530 × 10 15 m (rounded to the seven significant digits in the speed of light) found in several modern sources [10] [11] [12] was probably derived from an old source such as C. W ...

  6. SPT0615-JD - Wikipedia

    en.wikipedia.org/wiki/SPT0615-JD

    This distortion causes the light from the galaxy to arrive as an image lengthened to an arc of about 2 arcseconds long. [ 2 ] "JD" is short for "J-band Dropout" (the galaxy is not detected in the so-called J-band (F125W) [ 4 ] The observed image is of 13.3 billion years ago, indicating the galaxy existed when the universe was about only 500 ...

  7. Parallax in astronomy - Wikipedia

    en.wikipedia.org/wiki/Parallax_in_astronomy

    A parsec is the distance from the Sun to an astronomical object that has a parallax angle of one arcsecond (not to scale). The parsec (symbol: pc) is a unit of length used to measure the large distances to astronomical objects outside the Solar System, approximately equal to 3.26 light-years or 206,265 astronomical units (AU), i.e. 30.9 trillion kilometres (19.2 trillion miles).

  8. Luhman 16 - Wikipedia

    en.wikipedia.org/wiki/Luhman_16

    Luhman 16 (also designated WISE 1049−5319 or WISE J104915.57−531906.1) is a binary brown-dwarf system in the southern constellation Vela at a distance of 6.51 light-years (2.00 parsecs) from the Sun.

  9. Epsilon Indi - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Indi

    Epsilon Indi, Latinized from ε Indi, is a star system located at a distance of approximately 12 light-years from Earth in the southern constellation of Indus.The star has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.674. [2]